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A NNALES DE L ’I. H. P., SECTION A

G. F. D ELL ’A NTONIO

Large time, small coupling behaviour of a quantum particle in a random field

Annales de l’I. H. P., section A, tome 39, n

o

4 (1983), p. 339-384

<http://www.numdam.org/item?id=AIHPA_1983__39_4_339_0>

© Gauthier-Villars, 1983, tous droits réservés.

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http://www.numdam.org/

(2)

339

Large time, small coupling behaviour

of

a

quantum particle in

a

random field

G. F. DELL’ANTONIO

Istituto di Matematica G. Castelnuovo, Universita di Roma Inst. Henri

Vol. XXXIX, 4, 1983,

Section A :

Physique theorique.

SUMMARY. - For a quantum mechanical

particle

in a suitable random field we prove that all finite-dimensional distributions of extensive obser- vables converge in the Van Hove

limit

to the

corresponding

distributions of a classical Poisson process. In the classical limit this process converges to a diffusion.

RESUME. 2014 On

demontre,

pour une

particule quantique

dans un

potentiel

aleatoire

convenable,

que toutes les distributions de dimension finie d’obser- vables extensives convergent dans la limite de Van Hove vers les distri- butions

correspondantes

d’un processus de Poisson

classique.

Dans la

limite

classique,

ce processus converge vers un processus de diffusion.

1. INTRODUCTION

The motion of a classical or quantum system in a random environment is

expected

to converge to a Markov process under suitable

scaling limits, usually involving large

time scales and small

coupling.

Results in this

direction appear in the literature under various

headings,

e. g.

homogenei- zation, method

of average, diffusion

limit,

and

require

in

general

detailed

specifications

as to what constitutes a random environment and which

are the observable

quantities

to be studied.

_ Formal results and

applications

can be

found,

e. g., in

[1 ].

The

subject

has also been considered in the mathematical

literature ; general

results

Annales de l’Institut Henri Poincaré-Section A-Vol. XXXIX, 0020-2339/ 1983/339/$ 5,00/

(0 Gauthier-Villars 13

(3)

340 G. F. DELL’ANTONIO

can be found in

[2 ],

where one considers the case in which the interactions with the random environment are a

priori

assumed to be

weakly

correlated

in time. These results can be viewed as a version of the central limit theorem for a class of

dynamical

systems.

A more

physical setting

is one in which the random force field is assumed to have weak correlations in space, to

reproduce

the

properties

of a

rapidly fluctuating

environment. In this case, the fact that successive interactions

are

weakly

correlated in time becomes part of the

proof (and

indeed

usually

the most difficult

part);

once this is

established,

the results follow modulo

(often

very

substantial)

technical details. This more

physical setting

is

beyond

the reach of the

general

results in

[2 ],

and

proofs require

the

develop-

ment of

specific techniques.

For

example

in

[3] it

is

proved,

under suitable but rather weak assump-

tions,

that the

velocity

process of a classical

particle moving

in a random

force field converges

weakly

to a diffusion process in the limit in which the force field becomes

(locally)

infinitesimal and the time scale is chosen

indefinitely large (Van

Hove

limit).

Here we prove a similar result for the motion of a quantum

particle

in

a random

potential

field.

As in the classical case, convergence will hold

only

for a restricted class of

observables,

in

particular

for bounded continuous functions of momentum.

Results in this direction are contained in a

germinal

paper

by

L. Van Hove

[4 ]. Important

steps and

proofs

are in

[5 ], [6 ].

The

limiting

process is here a Poisson process, with transition

amplitudes depending

on Planck’s constant ~.

It is a rather obvious

question

to

inquire

whether the results of

[3] ]

for the classical case can be recovered in the classical limit. This is indeed the case ; in the last section of this paper we shall

briefly

indicate the way in which a

proof

is

given.

A full

proof

will be contained in

[10 ].

It should be noted that the results we present here for the quantum case

are obtained under conditions on the force field which are stronger than those of

[3 ].

The results themselves are moreover weaker than their classical counterpart, in so far as we

only

prove convergence of all finite-dimensional distributions rather than convergence of processes. The

assumptions

are stronger both because the force field is taken to be

potential -

this seems

unavoidable in

Quantum

Mechanics - and to admit moments of all

orders,

with suitable bounds in terms of the moment of order two. Some restrictions on the bounds can be lifted

by

more accurate

estimates,

but

our method of

proof

does not

exploit enough

the details of the quantum mechanical evolution on the

space-time

scale characteristic of the

problem.

In the classical case, many estimates

depend

on a rather detailed

description

of « most »

trajectories;

that the Poisson process of the quantum case

Annales de Henri Poincaré-Section A

(4)

341

A QUANTUM PARTICLE IN A RANDOM FIELD

converges as a process to the diffusion of the classical case suggests that also in the

quantum-mechanical setting

it should be

possible

to have

a better control of the « motion of the wave

packet »

for most

configurations

of the force field.

It seems however that the main drawback of the method

presented here,

both in terms of

assumption

needed and of results which can be

obtained,

is to be found in the fact that we are able to use

only

a very modest amount of

probabilistic techniques.

In

particular

we lack the

inequalities

for conditional

expectations

and the

resulting tightness

of a suitable

family

of

probability

measures, which are the main tool in the

analysis given

in

[3 ],

for the classical case.

A better strategy of

proof

could come from a more

probabilistic approach

to the

quantum-mechanical

case, for instance a formulation of the motion of a quantum

particle

in a

potential

field in terms of

integrals

over suitable

functionals of a Poisson process, as

developed

in

[8 ].

In this case, it is conceivable that a « small » set of

trajectories

will

give

the dominant

contribution in the Van Hove

limit,

and that the

techniques developed by

Donsker and Varadhan

[9] ]

could put to use here.

We are indebted to Ph. Combe for some very

suggestive

discussions

on this

possibility.

The content of this paper is as follows.

In this section 2 we

give

some further

qualitative

comments and the

description

of the quantum mechanical evolution of a suitable class of observables in a

properly

defined random

potential

field.

In section 3 we

provide

motivations and describe the limit Markov process.

In section 4 we

begin

the

proof

of convergence of the

averaged dynamics

when the

potential

is a Gaussian random field and outline the strategy;

further technical details and the

completion

of the

proof

are

given

in

section 5.

In section 6 we outline the

proof

of convergence for all finite-dimensional distributions. We also outline how the

proofs

can be extended to cover

the case of random

potential

fields which are not

gaussian.

In section 7

we prove that the Markov process described in section

3,

converges, when ~ -~

0,

to the diffusion process of the classical case.

2.

QUANTUM

EVOLUTION

IN A RANDOM HOMOGENEOUS POTENTIAL FIELD Let

V(x)

be the

potential

field. The motion of a quantum

particle

is

described

by

the

Schrodinger equation

Vol. XXXIX, 4-1983.

(5)

342 G. F. DELL’ANTONIO

when A =

/ ~2 ~x2i, 03C8

E

L 2(1R3)

n

D( - h20394

+

V),

and for convenience we 1

have taken units of mass such that m ==

1/2.

We shall consider

only

motion in

1R3, although

all the results we state also hold &#x3E;

3,

and in fact some of the

proofs

in

§ 4,

5 become

simpler.

Some crucial estimates in

§ 4, 5

fail instead for n == 1 or

2,

as will be apparent in the

sequel.

The result could still be true for n =

2,

which is somewhat

a borderline case, but the method of

proof

we present here fails in this

case. Since h

plays

no role until

§ 7,

we shall set h = 1 until then.

In order that

(2.1) provide

a

unitary

evolution in

L 2([R3)

it is sufficient

by

Stone’s

theorem,

that - A + V be

self-adjoint.

If this is the case, let be the

corresponding

one-parameter group of

unitary

operators ;

one has = exp

i( -

1B +

V)t.

Let B be a

symmetric

bounded linear operator on

LZ(f~3),

i. e. a quantum mechanical

observable ;

its time

evolution,

in the

Heisemberg representation (which

we shall

adopt)

is

given by

Let

R3

E a -H-

V(a), (V(~)~)(~) = .p~ - Q)

be the standard

representation

of the group of

space-translations.

We shall denote

by ~o

the linear span over the

complex

numbers of

the observables which commute with for

all a

E

R 3. j~o

is

easily

seen

to be a commutative C*

algebra,

which can be identified via Fourier transform with the

algebra

of

essentially

bounded functions on [RP.

Indeed,

if A E one has

for some function

A(p_)

E

L 00([R3). Here ~

is the Fourier transform of

1/1.

We shall call this the Fourier

representation

of

Ao.

Denote

by Co(R 3)

the class of continuous functions which vanish at 00; is a

subalgebra

of

L 00,

closed in the supremum norm. Let s~ be the

subalgebra

of

j~o

which has as

representative

in the Fourier

representation;

~ is

then closed in the norm

topology.

The observables for which we shall prove limit theorems are the

symmetric

elements of j~.

We recall now

briefly

the definition of a random field. Let Q be a

proba- bility

space, with

generic point

~ endowed with the measure ,u. Let S be

a linear

subspace

of

C(R 3; R) (continuous

functions from

R3

to

R)

and

let S 3

f ~

be a linear map from S to the linear space of random variable

(~-measurable

functions over

Q).

Formally,

one writes ,, t/

where for

co)

is a

(generalized)

function of jc. In favourable

Annales de l’Institut Henri Poincaré-Section A

(6)

343

A QUANTUM PARTICLE IN A RANDOM FIELD

cases,

úJ)

will be for each x a random variable. For a measurable and

integrable

function on

Q,

we define ,

We

require

that V be

stationary

and

ergodic.

The field

V(x)

is

stationary

if

for

all a

E

[R3,

as elements of

(S*)n,

S*

being

the dual of S.

One can choose Q in such a way that there exists a

representation

of

R3 by unitary

operators

Ta

on

L 2(0, ,u)

such that

Ergodicity implies

that every measurable function of the random field

V,

which is invariant under

Ta

differs from a constant function

only

on

a set of ~-measure zero.

If E(V(xl)

... exist as continuous

functions,

then for each x~

1R3,

is a random

variable,

and one can choose a modification

(on

a set

of zero

measure)

of such that the

resulting

field

is jointly

measurable

in x and úJ.

These conditions are in

particular

met

if V(x)

is a centered

( =

mean

zero)

Gaussian field of covariance

~(ç),

where G is continuous. One has then of course

We shall state our results and

give proofs only

in the case in which

V(x)

is a Gaussian random field. As will become apparent in the course of the

proofs,

the results can be extended to more

general

random

fields, provided

one has suitable a

priori

bounds on the moments of V.

On the Gaussian random field V we shall make the

assumption.

ASSUMPTION A. -

If |g|1

is the L 1 norm

of g,

we shall use the notation

Having

thus set our

notation,

we

begin constructing

the evolution of the observables in j~ under the influence of the random

potential

field V.

In the Gaussian case, it is not difficult to prove that there exists a set

Qo

of measure one, such

that,

if úJ E

03A90, H( úJ) == - 1B

+

co)

is

essentially self-adjoint

on

CÜ(1R3).

This is sufficient to define a

dynamics

for a . a . cc~.

We shall however be interested in

regularity properties

of the average

Vol. XXXIX, 4-1983.

(7)

344 G. F. DELL’ANTONIO

dynamics.

To obtain

these,

we choose to

approximate

first and

to define the

dynamics by

a

limiting procedure.

A natural choice would be For all x, ~ is bounded

below, uniformly

in x, co. If it follows from the individual

ergodic

theorem that

for a . a . cc~,

VE1~( ~, cc~) E L o~(~3),

the space of functions which are in L2 when restricted to any bounded subset of

[R3.

Therefore there exists a set

03A91

c

Q, (03A91)

=

1,

such

that,

if

- Ll +

VE1~( ~,

is

essentially self-adjoint

on

CÜ(1R3).

Moreover

is a core for - 0394 +

V(1)~, and exp i(- 0394

+

V(1)~(., 03C9))t is strongly

continuous

in t for all cc~ E

Q,

and

strongly

measurable in cc~ for all t

(this

can be

proved,

e. g.,

using

the Trotter

product formula,

since the

pointwise

limit of measu-

rable functions is itself

measurable).

While

(2. 5)

is in many ways a natural

approximation,

it

requires

much

machinery

to prove

that,

for all t E

R,

úJ E

03A91,

the limit ~~0 exists as a

unitary

operator.

We shall choose therefore the

following approximate

random field Since is

jointly

measurable in

(x, a~),

so is Moreover

by construction, V(x, úJ)

is bounded

uniformly

in

(x,

We will prove

LEMMA. 2014 For

each t, 03BB

there is a

set Q

c

Q, (03A9)’

==

1,

and a sequence ~n,

8n ~ 0 when ~ -~ oo, such

that,

if úJ E

Q,

strong

limit

+

exists. Call this limit.

_

Then

U~(~)(~)

is

unitary

for all úJ E Q and

~-measurable.

D

Proof

2014 We shall prove

that,

for

every ~

one has

Assuming

for the moment the

validity

of

(2.7),

we

complete

the

proof

of the Lemma.

be a denumerable basis in

L 2([R3).

From

(2.7),

is,

for each K =

1, 2,

... a

Cauchy

sequence in

L 2([R3

X

Q, v),

where

v = ,~~ x ,u and is

Lebesgue’s

measure on [R3. It then follows

that,

for

each K E Z + there is a set

= 1,

and a

subsequence 0,

such

that,

for all cc~ E A +

~K

converges in

Let Q = Therefore = 1.

KEZ+

Annales de l’Institut Henri Poincaré-Section A

(8)

345

A QUANTUM PARTICLE IN A RANDOM FIELD

One can choose a

sequence ~n ~

0 such

that,

if 03C9 E

Q,

converges in for all

(the sequence {~}

is a

subsequence

of

each { ).

Since + is norm-bounded

uniformly

in 8,

converges in for

all 03C8

E as can be seen

approximating 03C8

with

finite linear combinations of the Let be the limit

point.

From

(2 . 7)

it follows

that 03C8 ~ ~03C8(03C9)

is linear and

bounded,

and in

fact ~~03C8(03C9)~ = II 03C8 II I (all

norms

being L 2([R3) norms)

since the unit

sphere

is closed under sequen-

tial strong convergence. _ _ _

Therefore for

each t, aL

there exists a

set

Q c

Q, ~(Q)

= 1

(the

set Q

depends

in

general

on t,

03BB)

such

that, if 03C9~03A9,

there exists a

unitary

operator which is the strong limit of + t.

Measurability

of follows since it is the

pointwise

limit of measurable functions.

It remains therefore to prove

(2.7),

which in turn is

equivalent

to

We shall use the

following identity,

where the series is norm convergent for all ~ &#x3E; 0 and úJ E

Q, uniformly

in co.

We shall refer to

(2.8)

as «

Dyson

series ». Notice that the left-hand of

(2. 8)

satisfies the differential

equation

where

V,(t)

=

The series

(2. 8)

is obtained

by iterating

the

integrated

version of

(2.9),

also called Duhamel’s

formula,

or « variations of constants ».

Substituting (2. 8)

in

(2. 7’)

one sees that one must

study

the limit when

~

~ 0 of

Vol. XXXIX, 4-1983.

(9)

346 G. F. DELL’ANTONIO

(the exchange

of the summation over m, n and

integration

over ti, Tj is

legitimate

in view of the boundedness of the The

integrand

can be

expressed

as a formal series

Let Eo = max

(8, 8’). Using

the

properties

of the Gaussian

integrals,

we shall prove that

380

such

that,

for Eo

Eo,

the series

(2.11)

is

absolutely

convergent,

uniformly

in 80. From this result

(2. 7’) follows,

since it is

easily

verified that

(2.10)

has no terms of order zero in Eo.

In

particular,

one has

and the sum is over all unordered

pairing

of the

points {xi},

each of which

is taken with

multiplicity 2KI

+ 1. In

(2.12), Kmn E Z+

is the number of

the times the

point

xm is

paired

with the

point

xn.

By carrying

out

explicitly

all calculations one verifies that each

integrand

in the serie

(2.10) gives

a contribution which is bounded in absolute value

... Y ..

by ~ A~2~j~1

1

j= 1 2 11.p 112 independently of t

1 ... zm. The inte-

gration

over t 1 ... 2m

provides

for each such term a factor

tn + m(n !) -1 (m !) -1.

To prove absolute convergence of

(2.11), uniformly

in 0 ~ is

therefore sufficient to prove absolute convergence of the series

where represents the number of

pairing

among n + m

points

xi, i == 1 ... n + m, each taken with

multiplicity Ki,

and we have set

= ~

~=1...~.

To evaluate

N,

it is easier to count

pairings

in a somewhat different way.

Annales de l’Institut Henri Poincaré-Section A

(10)

347

A QUANTUM PARTICLE IN A RANDOM FIELD

Let

Kij i, j

= 1 ... n + m be the number of times the

pair (i, j)

appears in the

pairing. Obviously

The number of

pairing

is then

We rewrite then

(2.13)

as

We now use the fact

that,

if

(2.13) holds,

then

and repeatedly

Schwartz’

inequality

to dominate the series in

(2.16) by

where 2K, + 1 == 2K.. + K,;.

Now,

and

moreover

Therefore

(2.17)

is dominated

by

Vol. XXXIX, 4-1983.

(11)

348 G. F. DELL’ANTONIO

which is

absolutely

convergent

uniformly

in

/),,

~ over bounded sets for

Bo2-5!2(11~lll)-1.

D

We are

mostly

interested in the random evolution of quantum observables.

This is

again

defined

by

a

limiting procedure.

Let

We have

THEOREM 1. 2014 For

each t,

~, there is a set Q c

Q, ~u~) - 1,

and a sequence 0 such

that,

if 03C9~03A9 and strong

limit A~n,03BB(t, úJ)

exists. Call the limit. Then A -~ is for each úJ a

unitary isomorphism

of A with a

subalgebra of B(L 2([R3)).

Moreover is

weakly

,u-measu- rable for

each t,

/).

and,

for

Proof -:-

A part from

measurability

and

(2 . 20),

all

remaining

statements

of Theorem 1 follow from Lemma

1,

and moreover one has

To prove the

remaining

two statements, it suffices to prove

that,

for

any

given A E ~, ~ E L2(~3), ~,,

t E R.

Indeed,

from the strong convergence of to

A~{t,

for

and Schwartz’s

inequality,

one concludes that for

every ~

E

L 2(1R3) (03C8, A~n,03BB(t)03C8)

converges in

,u)

to

(1/1, A03BB(t)03C8)

and this

implies

measurabi-

lity and (2.20).

The

proof

of

(2.21)

follows the same lines as the

proof

of

(2.7).

One

starts from the

Dyson series,

obtained

by iterating

the

integral

version

of the

equation

where

A£,~(t) -

The

Dyson

series for observables is

a norm convergent series in view of the definition

ofV,.

The

proof

of

(2.21) given (2 . 22)

follows then the same steps as the

proof

of

(2 . 7)

in Lemma 1,

and we shall not repeat the details here. D

Annales de Henri Poincaré-Section A

(12)

349

A QUANTUM PARTICLE IN A RANDOM FIELD

Remark. 2014 Notice that Theorem 1 and its

proof provide

also an

explicit

formula for

E(.p,

One has indeed

From the

proof

of theorem 1 it also follows

COROLLARY. For every choice

of t 1,

..., tn, ~, there is a set

Q’,

==

1,

and a

sequence ~n ~ 0,

such that if co E Q’ and E A i = 1 ... n, the

strong limit of

AEm},~(tl) ~ ... ~ AEm~,~(tn)

exists and coincides with

Moreover the latter operator is

weakly

measurable in co, and

for D

- Since the

are uniformly bounded for

£ 0 and

weakly measurable,

the operators = and

A~)

=

E(A~(~))

are well defined and

belong

to

j~o

since the process is

stationary.

Similarly, ... ~ A~,n~(tn)) E ~o,

but it is of course different from

A~,l ~(t 1 )

...

We now prove that all these operators are in fact in j~. Indeed one has

LEMMA 2. - For all choices ...

and

is jointly

continuous in the

tk’s.

In

particular

the average

dynamics

A ~

A~(t)

is defined in j~ and continuous in t. D

Proo, f.

shall

give

the

proof only

for n = 1. A part from notational

complications,

there is no

difficulty

in

extending

the

proof

to the

general

case.

From

(2.22)

one obtains in the Fourier

representation

Vol. XXXIX, 4-1983.

(13)

350 G. F. DELL’ANTONIO

where po == pn = ~ and the third sum is over all

permutations K iK

such that

tiK+

1 if

K hand tiK tiK+

1 if K &#x3E; h.

The estimates

given

in the

proof

of Lemma 1 can then be

applied

to

(2 . 25) (there

is an extra factor 2" in the

estimates, coming

from ;

indeed

this

perm

sum

corresponds

to

summing

over the 2n terms in the

multiple

commutator

which

appears

in

(2. 22))

and

they

are uniform in

Therefore converges to

A03BB(t)

in norm

(recall

that for

each 03C9~

one had

only

strong

convergence)

and it remains to prove that E j~.

By

the same estimates as

above,

the series

(2. 25)

is

absolutely

convergent

uniformly in p,

and therefore it suffices to prove that .each term

belongs

to ~.

Each term in

(2.25)

with h ~

0, n

can be put in the form

where K n C

(and depends parametrically on ~,, t),

while the terms

with h = 0 or n

(and

therefore ph =

p)

are of the form where

K 1

is a bounded continuous function

of p.

Since A E

~, clearly K 1

A E j~.

To prove that E ~~, notice first that

B(/?)

is continuous, since K E L 1.

Indeed, for all

y, ; y ;

&#x3E;

0

and N &#x3E; 0 one has

,

and this

expression

can be made

arbitrarily

small

by

first

choosing

N

sufficiently large

and

then I ~ I sufficiently small, using

the

continuity

To prove

that lim B(p)

=

0,

notice

that,

since A E

~, given ~

&#x3E; 0

-

~

there exists

such

that if p ~

&#x3E;

M£, where K 11

is the L2-norm of K.

-

1

-

One has

then, for 1£

&#x3E;

Nt

+

Mt

since,

if

I

Ne and 1£

&#x3E;

Ne

+

then 1£ - £’

&#x3E;

Me.

Q

Annales de l’Institut Henri Poincaré-Section A

(14)

A QUANTUM PARTICLE IN A RANDOM FIELD 351

It follows from Lemma 2 that A ~ is a linear continuous map of A into itself. It is

given explicitely

in

(2. 23)

as a norm-convergent power serier in

/L,

but it is in

general

not differentiable

in t;

even for those A E j~

for

which differentiability

can be

proved,

no

simple equation

will be satisfied

by A;.(t).

. _

We shall however prove in

94

that

A;.Cr/Å2)

converges, when ~, ~

0,

to a Markov

semi-group

with continuous parameter r.

3. SOME PROPERTIES OF THE EVOLUTION IN

THE LIMIT

t = ~/~,2,

/~0

We shall

study

in

§

4 the limit t =

z/~,2, ~, ~

0 of the

averaged dynamics

and of all correlation functions.

Here we

provide

some motivation to indicate which is the limit to be

expected,

and we

study

the convergence of a sequence of Markov processes

T).

somewhat related to the

averaged dynamics.

A part from

giving

some hints at the mechanism which will be put

at work in

§ 4,

we

give

here also some estimates which will be of use in the

sequel.

As a

preliminary

we shall

study

the operator

Obviously

Formally, A~~~/~,2~

satisfies the

equation

where

Ho - - 4.

This relation is

only suggestive,

since we have not

proved

that there

are cu E Q for which

A~(~

is

differentiable,

even if

only weakly.

We write

formally

and substitute in

(3.1), equating

terms of the same order in ~,. This leads to

The first relation in

(3 . 2)

is

compatible

with

A(0)(t, úJ)

E

A0

for all 03C9 ~

SZ1, although

it does not

imply

it. Due to the

ergodicity

of the process, one has then

A~°~(t,

=

E(A~°~(t))

for

Vol. XXXIX, 4-1983.

(15)

352 G. F. DELL’ANTONIO

From the second relation in

(3.2)

we conclude

then,

at a formal level

(since

= 0

1).

--

Equation (3.3)

is understood in the sense

that,

for

all 03C8

for which the

integral

converges for a. a .p,

where 03C8

is the Fourier transform

of 03C8

E

L 2(1R3)

and

V(/7, p’ ; 03C9)

is defined

We now substitute

(3.3)

in the third relation in

(3.2), again formally

since we do not control the domains of the generators

involved,

to obtain

We

integrate

over

Q,

and use the fact

that,

due to the

stationarity

of the

process,

E( [Ho, A(2)(T)]) == 0,

and moreover is

independent

of co on a set of measure one. One obtains

where

Therefore,

Remark. - This heuristic argument would suggest that a stronger result should be

expected, namely

that there is a set

03A91

c

Q,

=

1,

such that

for all 03C9~03A91.

We do not know if

(3.7’)

holds in a weak sense, with

Q1 depending

on T and on the vectors in which enter in the definition of weak convergence.

Certainly (3 . 7’)

cannot hold in a strong sense, since it would contradict the result we establish for

Annales de Henri Poincaré-Section A

(16)

353

A QUANTUM PARTICLE IN A RANDOM FIELD

The derivation of

(3 . 7) given

above is at best

heuristic,

as evident from the remark above.

Still, (3 . 7)

is correct, as we shall prove in

94.

We shall do so

by approximating E(A;.(T/Â2) by

the solution

A~(r)

of

a suitable linear

equation.

In

g4

we shall prove that

E(A~(T/~)) 2014

converges to zero in the

topology

of j~ when )" ~ 0. Here we shall define

A~(r)

and prove

that, again

in the

topology

of

~,

converges to when ~ -~ 0.

We

begin by noting

that

when

~ÀCr/)~2)

= exp

T/À2)AÀ(T/)~2)

exp

( - i~~/~~2)

and

that, according

to

(2 . 23)

where

From

(3.9)

one should expect ~ 0 when /t -~

0,

due to some mild

mixing properties

of the process and the local

decay

of for

large

t.

Indeed,

this is what is

proved

in the classical case,

using a priori

estimates for conditional

expectations

and some information on the

properties

of « most » classical

trajectories.

We shall prove

in § 4

that

D~(~)

~ 0 in the

topology

of j~. Motivated

by this,

we define to

be the

(unique)

solution of

Notice that is « sure », i. e. it does not

depend

on co.

Eq. (3.10)

can be solved

by iteration,

which

provides

a norm convergent series for all

~,,

T. The solution is therefore

unique,

and this proves that

since,

if

A{ 1 ~(z)

is a

solution,

so for

In the Fourier

representation

one has

explicitely

Let J~f be defined as in

(3.6)

and let exp - ~t be the

semi-group

it generates

(the

existence of

exp ( -

is part of the

proof

of the next

lemma).

Vol. XXXIX, n° 4-1983. ~ ,

(17)

354 G. F. DELL’ANTONIO

One has then

LEMMA 3. 2014 For all and r ~

0, A(T) - e - ~z.

A converges to zero, when ~, ~

0,

in the

topology

of j~. D

Proof

2014 From

(3.11)

it is

easily

seen

that

for some 0.

We write

(3.11)

in

integro-differential form, taking

the derivative with respect to T, and then take

Laplace

transform.

For ,u

&#x3E; Yo, define

From

(3.11)

one has

with

As a linear operator on

~0(~3), ~~,;,~

is accretive for all ,u &#x3E; 0.

Indeed,

if

f

E

Co([R3),

let

p_o

be a

point

at

which

reaches its maximum

(all

our

function spaces are

real).

Let lf

be the element of defined

by

= We prove

that 0.

Indeed,

notice that == 0 =&#x3E;

f

=

0;

assume then

0. Then

Since, by

definition of

/(~o)) ~

0 VK E

[R3,

one has

indeed

!/~/) ~

0

-

Since ~ is

bounded,

range

(~

+

~o) _

for

~,o sufficiently large.

We conclude

that ~~

is accretive for every ,u &#x3E; 0. Therefore its spectrum is contained

in {ç Re 03B6 0}

and we can

define,

for

all

&#x3E;

0,

Clearly A~

=

A~;~

at least

for ,u

&#x3E; ~ since

A~;~

is

analytic

for

0,

it follows that

A03BB(t)

has a

Laplace

transform

for

&#x3E;

0,

and

A03BB; = A03BB,

&#x3E; 0. Let be defined

by

=

(2 -

/~’

I) -1 A{ p) ;

since ~ is

accretive

(the proof

is

given

as

above) A~~~{p)

is well defined for all ,u, Re ~c &#x3E;

0,

and is in fact the

Laplace

transform of

From

(3.15),. (3.14)

The

right-hand

side converges to zero in the

topology

of

~ ; since,

for

,u &#x3E;

0,

I -

~~,,~)

is bounded away from zero

uniformly

in ~, &#x3E;

0,

we conclude

A03BB, - A( ) ~

0 for

all

&#x3E;

0, uniformly

in 0 ð ,u N.

Annales de l’Institut Henri Poincaré-Section A

(18)

355

A QUANTUM PARTICLE IN A RANDOM FIELD

From this it follows that

A~) -

0 in the same

topology.

D

Some information on the structure of the limit

semi-group Tt

=

~~

is

provided by

the

following

LEMMA 4. - The

semi-group Tt

is a contraction

semi-group

on j~.

It is reduced

by

each ball

Ba3~ : ~ p ~ ~ p ~ I a ~

and defines on each

sphere S~3) : {£ I I p I == ~ }

a contraction

semi-group.

On each

sphere,

the constant

function is left invariant

by T~.

Proo, f :

have

already proved

that 2 is accretive. Therefore

Tt

is

a contraction

semi-group. Next,

we notice

that,

if

f

E has support contained

a p ~ b ~

for some

a, b

&#x3E;

0,

then

Ttf

has support contained in the same set. This is evident from the definition of

J?,

and

the fact that is

given by

a norm-convergent series in t.

Consider now on

(continuous

functions on the

sphere

of radius

one in

1R3)

the

family

of operators

where a &#x3E; 0 and

p) _ ap).

One verifies

easily that,

for

all f

E

where ~

f a(~) _ ,

The operators

2 a are accretive for every a

&#x3E; 0. Let be the associated

semi-group.

From

(3.18)

one verifies that

in the natural

decomposition

of

Cü([R3B0)

as a

subspace

of

0

Constant functions on are left invariant

by

since

~a ~

1 - 0. D Assume now

that a

satisfies for every a &#x3E; 0 a strong form of Doeblin’s

condition,

i. e. for

every ~

E

Sa3~,

B c

Sa3~, ~an~( p,

0 for some

B

cient condition for this to hold is that

~(~)

has compact support, or exponen- tial

decay.

One has then

COROLLARY. 2014 Under the condition stated

above,

the constant function

on is a

global

attractor for the

semi-group Tt.

Given any function

Vol. XXXIX, 4-1983.

(19)

356 G. F. DELL’ANTONIO

g E

Co, Ttg

converges when t -~ oo

towards g,

where

g

is a function

only

Proof

2014 Under the stated

conditions,

1 is the

only eigenvector

of

T~a~

to the

eigenvalue

zero. The

corollary

follows then from standard

properties

of contraction

semi-groups.

D

2014 The

physical description

behind Lemma 4 is that the random force

field,

in the limit in which ~, ~

0,

does not alter

appreciably

the

energy of the

particle,

even if it acts for a time of order

~,- 2.

On such a

long

time scale however the momentum of the

particle undergoes changes,

in such a way

that,

on a still

longer

time scale

(r

~

oo),

its distribution becomes uniform on the mass shell.

4

CONVERGENCE

TO THE MARKOV LIMIT:

CONVERGENCE OF DYNAMICS

Let be defined as in Theorem

1;

in this section and in the

following

we shall

study

the limit of ,

when ~, -~

0,

when E j~ i = 1 ... n, and T 2 ~ ... ~ In this section we consider the case n =

1,

and prove

where

T,

is defined as in

(3.7), (3.6).

This will be the content of Theorem 2.

Before

stating

the theorem

precisely,

we

perform

some

preliminary operations

and prove two lemmas which will be used in the

proof

of

Theorem 2.

From

(3.8), (3.10)

it follows

that, setting

where is defined as in

(3.9)

If one can prove that

D~r) -~

0 when}1. ~

0,

then

(4.1)

follows from

Lemma 3 and an

application

of Gronwall’s

inequality.

If one had for the present

quantum-mechanical setting

the definitions

-

Annales de l’Institut Poincaré-Section A

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